Macías-Pérez, J.F., Adam, R., Ade, P. ![]() ![]() ![]() ![]() ![]() |
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Abstract
Clusters of galaxies, the largest bound objects in the Universe, constitute a cosmological probe of choice, which is sensitive to both dark matter and dark energy. Within this framework, the Sunyaev-Zel’dovich (SZ) effect has opened a new window for the detection of clusters of galaxies and for the characterization of their physical properties such as mass, pressure and temperature. NIKA, a KID-based dual band camera installed at the IRAM 30-m telescope, was particularly well adapted in terms of frequency, angular resolution, field-of-view and sensitivity, for the mapping of the thermal and kinetic SZ effect in high-redshift clusters. In this paper, we present the NIKA cluster sample and a review of the main results obtained via the measurement of the SZ effect on those clusters: reconstruction of the cluster radial pressure profile, mass, temperature and velocity.
Item Type: | Article |
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Date Type: | Publication |
Status: | Published |
Schools: | Physics and Astronomy |
Publisher: | EDP Sciences |
ISSN: | 2100-014X |
Date of First Compliant Deposit: | 10 March 2020 |
Date of Acceptance: | 27 January 2020 |
Last Modified: | 03 May 2023 22:50 |
URI: | https://orca.cardiff.ac.uk/id/eprint/130293 |
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